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• W2086036737 abstract "Estimates of the bombarding energies necessary to reach the quark-gluon phase in heavy-ion collisions are presented within a hydrodynamical framework. At intermediate energies (3-7 GeV/nucleon) the quark-gluon matter formed is predicted to be rather cool (below 100 MeV), i.e. much colder than nuclear matter without phase transitions. Further, the consequences of first-order phase transitions from the neutron matter to pion-condensed matter and quark matter are discussed for neutron stars. Quark matter does not fulfil the conditions for the existence of a third stable branch, e.g. stars with quark cores. Because of observational constraints on neutron-star masses, pion condensation is restricted to a narrow first-order phase transition at best. Due to this restriction the rapid growth of a pion-condensed core in a neutron star cannot appear as a supernova-like event as suggested in earlier work." @default.
• W2086036737 created "2016-06-24" @default.
• W2086036737 creator A5005010414 @default.
• W2086036737 date "1983-12-01" @default.
• W2086036737 modified "2023-09-24" @default.
• W2086036737 title "Phase transitions in dense nuclear matter and consequences for neutron stars" @default.
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• W2086036737 doi "https://doi.org/10.1088/0305-4616/9/12/009" @default.
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